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Massive Star Forming Regions in the Galactic Plane: A Comparative Study Using BGPS, Spitzer, & Optical/Near-IR Surveys

Published online by Cambridge University Press:  21 October 2010

Guy S. Stringfellow
Guy S. Stringfellow
Affiliation:
CASA, University of Colorado, 389 UCB, Boulder, CO, USA, [email protected]
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Abstract

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The Bolocam Galactic Plane Survey (BGPS) is a 1.1 mm continuum survey that has detected more than 8300 clumps over a 170 square degree survey area in the Galactic plane. The full power of these data is realised only when considering the full complement of data spanning millimetre through x-ray wavelengths.

Keywords

Galaxy: structureISM: jets and outflowsISM: structurestars: formationsurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 805
Copyright
Copyright © International Astronomical Union 2010

References

Aguirre, J. et al. 2009, ApJ Suppl in pressGoogle Scholar
Rosolowsky, E. et al. 2009, ApJ Suppl in pressGoogle Scholar
Schuller, F., Menten, K. M., Contreras, Y., et al. 2009, A&A in pressGoogle Scholar